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«Открытие космологических гравитационных волн в эксперименте по

«Открытие космологических гравитационных волн в эксперименте по измерению поляризации» M .В.Сажин 21 марта 20 14 ГАИШ Москва Россия. Fluctuation in the Universe.

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«Открытие космологических гравитационных волн в эксперименте по

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  1. «Открытие космологических гравитационных волн в эксперименте по измерению поляризации» M.В.Сажин 21 марта 2014 ГАИШ Москва Россия

  2. Fluctuation in the Universe • Our Universe is isotropic and homogeneous, but tiny perturbations exist. They are scalar (density perturbations) and tensor (cosmological gravitational waves). • Zeldovich Ya. in 1972 put forward a hypothesis about the initial state of our Universe and its perturbation from very general assumptioms.

  3. Harrison-Zeldovich spectrum • The paper MNRAS (1972), v.160, 1P Ya.B.Zeldovich predict a spectrum of fluctuation inour Universe which is called now Harrison-Zeldovich spectrum. 20 years later this magic prediction was confirmed by the observation of anisotropy of the CMBR. Hope that this week it was also confirmed by the polarization observation of the CMBR.

  4. Cosmological Gravitational Waves • Grishchuk, L. 1974 – parametric mechanism of graviton creation • Starobinsky, A. 1979 – graviton creation in the early Universe with f(R) gravitation • Rubakov, V.; Sazhin, M.; Veryaskin A. 1982 – graviton creation in the early Universe and Grand Unification Scale

  5. Equation of anisotropy produced by perturbations

  6. Polarization of the CMBR Stocks parameters:

  7. Polarization of the CMBR Incident light Scattered light Basko, M., Polnarev A., 1980;

  8. Anisotropy and Polarization

  9. Anisotropy and Polarization • Therefore one may resolve this equations and obtains and • Sazhin, M. 1984; Sazhin, M., Benitez, N. 1995; • Sazhin, M., Toporensky, A., 1995,1996; • Sazhin, M., Shulga, V., 1996.

  10. Multipole expansion of Polarization Sazhin, M., Shulga, V., 1996.

  11. Seljiak , U., 1997; Scalar perturbations do not produce B mode of polarization

  12. BICEP Experiment

  13. Gravitational waves from inflation generate a faint twisting pattern in the polarization of the cosmic microwave background, known as B-mode pattern. For the density fluctuations that generate most of the polarization of the CMB, this part of the primordial pattern is exactly zero. Here is the actual B-mode pattern observed with the BICEP2 telescope, which is consistent with the pattern predicted for primordial gravitational waves.

  14. Thank you for attention

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